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Electron-cyclotron maser radiation from a relativistic loss-cone distribution

Journal Article · · Phys. Fluids; (United States)
DOI:https://doi.org/10.1063/1.864542· OSTI ID:5305723
The electron-cyclotron maser instability is studied in a plasma with a loss-cone distribution for parameters relevant to tandem mirror devices. Both linear theory and particle simulations are employed. The effects of finite k/sub perpendicular/ are found to be very significant, and in general, the largest growth rate occurs for radiation emission perpendicular to the magnetic field. The instability persists at much lower densities (..omega../sub p/e/..cap omega../sub e/ < 0.1) than indicated by previous analyses, which were limited to the case of parallel emission.
Research Organization:
Department of Physics, University of California, Los Angeles, California 90024
DOE Contract Number:
AM03-76SF00010
OSTI ID:
5305723
Journal Information:
Phys. Fluids; (United States), Journal Name: Phys. Fluids; (United States) Vol. 27:10; ISSN PFLDA
Country of Publication:
United States
Language:
English